• 한국광학회지
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• 제30권4호
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• pp.146-153
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• 2019

노광기는 회로 패턴을 원하는 위치에 전사시켜주는 장비로 패턴을 광학적 특성의 변형 없이 기재 상에 나타내기 위해서는 노광광학계의 특성이 매우 중요하다. 따라서 미세회로 패턴을 형성하기 위해서는 조사 면적에 작은 발산각으로 입사되어야 한다. 또한, 광원에서 나온 빛이 감광제와 균일하게 반응해야 하기 때문에 높은 광효율과 조도 균일도를 가져야 한다. 본 논문에서는 협각 구현의 문제점을 해결하기 위한 방법으로 반사형 타입인 파라볼라 반사경과 비구면 렌즈 설계를 진행하였고, 배열 후 시뮬레이션 분석 결과 광속 각도, 균일도, 최대조도가 목표 성능을 만족하는 것을 확인하였다.

• 천문학회보
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• 제44권2호
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• pp.64.1-64.1
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• 2019

The first high-resolution spectroscopic and new multiband photometric observations of the semi-detached Algol type binary XZ CMi were performed at the Bohyunsan Optical Astronomy Observatory (BOAO) and the Sobaeksan Optical Astronomy Observatory (SOAO), respectively. A total of 34 spectra were obtained using the 1.8 m reflector of the BOAO equipped with the Bohyunsan Optical Echelle Spectrograph to construct the radial velocity (RV) curves of the eclipsing pair. New BVRI photometric light curves were also covered by using the SOAO 61cm reflector and a CCD camera. A detailed analysis of all eclipse timings shows that the orbital period of XZ CMi has varied in an upward parabolic variation superposed on a sinusoidal oscillation with a period of 38.0 yr and a semi-amplitude of 0.0071 days. From the spectral analysis, the effective temperature and the projected rotational velocity of the primary component were determined to be T_eff,1 = 7387±161 K and v₁sini = 122±6 km s^-1, respectively. Our simultaneous synthesis of the double-lined RV and BVRI light curves gives the reliable system parameters of XZ CMi with a mass ratio (q) of 0.314, an orbital inclination (i) of 81.9 deg and a large temperature difference (∆T) of 2481 K. The individual masses and radii of both components are M₁ = 1.91±0.08M_⊙, M₂ = 0.60±0.02M_⊙, R₁ = 1.60±0.02R_⊙, R₂ = 1.13±0.02R_⊙, respectively. Although the primary component is located inside the δ Sct and γ Dor instability strips, no evidence of pulsation in the system was detected. The possible evolutionary status of XZ CMi is discussed.

• 설비공학논문집
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• 제20권1호
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• pp.35-41
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• 2008

The radiative heat loss from a receiver of a dish solar collector is numerically investigated. The dish solar collector considered in this paper consists of a receiver and multi-faceted mirrors. In order to investigate the performance comparison of dish solar collectors, six different mirror arrays and four different receivers are considered. A parabolic- shaped perfect mirror of which diameter is 1.40 m is considered as the reference for the mirror arrays. The other mirror arrays which consist of twelve identical parabolic-shaped mirror facets of which diameter are 0.405 m are suggested for comparison. Their reflecting areas, which are 1.545 $m^{2}$, are the same. Four different receiver shapes are a conical, a dome, a cylindrical, and a unicorn type. The radiative properties of the mirror surfaces and the receiver surfaces may vary the thermal performance of the dish solar collector so that various surface properties are considered. In order to calculate the radiative heat loss in the receiver, two kinds of methods are used. The Net Radiation Method that is based on the radiation heat balance on the surface is used to calculate the radiation heat transfer rate from the inside surface of the receiver to the environment. The Monte-Carlo Method that is the statistical approach is adopted to predict the radiation heat transfer rate from the reflector to the receiver. The collector efficiency is defined as the results of the optical efficiency and the receiver efficiency. Based on the calculation, the unicorn type has the best performance in receiver shapes and the STAR has the best performance in mirror arrays except the perfect mirror.

• 한국인터넷방송통신학회논문지
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• 제11권3호
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• pp.9-15
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• 2011

리플렉트어레이 안테나는 반사경 안테나의 단점을 보완하여 대체할 새로운 형태의 안테나로 대두되고 있다. 하지만 반사판이 단층구조일 경우 대역폭이 매우 좁다는 단점이 있고, 대역폭을 넓히기 위하여 다층구조의 반사판을 사용할 경우 설계가 어렵고 제작 단가가 높아지게 된다. 본 논문에서는 이러한 단점들을 극복하기 위하여 단층구조를 사용하여 제작 단가를 낮추면서 협대역 특성을 극복할 수 있는 정사각형에 U자 모양 슬롯을 낸 패치를 이용하여 리플렉트어레이 안테나를 설계하였다. 제안된 리플렉트어레이 안테나는 12.5 GHz에서 55.5 %의 효율과 14 % 이상의 1 dB gain bandwidth 특성을 갖는다.

• 한국전자파학회논문지
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• 제27권5호
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• pp.471-481
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• 2016

밀리미터파 대역에서 동작하는 안테나의 성능 측정을 위한 컴팩트 레인지 설계 및 실험 결과에 대해 소개한다. 전기적 거대 구조인 컴팩트 레인지의 포물면 반사판에 의해 형성되는 측정영역의 평면파를 해석하기 위하여 물리광학 기법을 적용하였다. 제작한 밀리미터파 컴팩트 레인지는 측정영역 전계 분포 실험과 고이득 안테나 측정을 통해 성능을 검증하였다. 동작 주파수 75~110 GHz에서 측정영역 직경 50 cm를 갖도록 설계한 컴팩트 레인지의 전력 균일성은 0.75 dB 이하로 측정되었다.

• KIEAE Journal
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• 제6권4호
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• pp.11-16
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• 2006

This work has carried out some preliminary studies for the utilization of a solar mini-dish system capable of concentrating solar rays to higher densities. A typical mini-dish system considered employs an array of solar mini-dishes where major components are light and compact. It consists of small mini-dishes, optical fiber bundles and diffusers at the end. Each mini-dish (typically has a 20 to 30 cm in diameter) is designed with a simple parabolic profile, concentrating sunlight (after the glass glazing cover to avoid dust deposition on the reflector and facilitate cleaning) onto a centrally-located small mirror which is placed on the bottom side of the transparent glass cover. The focused sunlight is reflected by the mirror surface onto a focal point where the receiving aperture of a homogenizer is located. Optical fibers are used to carry high-density solar rays to the other end where diffusers are mounted for indoor illumination. The proposed high density mini-dish system could make an efficient daylighting system as it excludes large moving parts and expandable if necessary. Each component of the system could be made from the off-the-shelf technology and thus, make the generic unit inexpensive to manufacture. Depending on spatial demand or characteristics, the amount of introducing daylight could be controlled. Preliminary tests have been carried out for a trial system to check any functional problems when in operation. Suggestions are also made to improve the design enhancing its performance and applicability.

• Journal of Biosystems Engineering
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• 제38권1호
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• pp.41-47
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• 2013

Purpose: The objectives of this study were to construct the solar drying system with evacuated tubular solar collector and to investigate its performance in comparison with indoor and outdoor dryings. Methods: Solar drying system was constructed with using CPC (compound parabolic concentrator) evacuated tubular solar collector. Solar drying system is mainly composed of evacuated tubular solar collector with CPC reflector, storage tank, water-to-air heat exchanger, auxiliary heater, and drying chamber. Performance test of solar drying system was conducted with drying of agricultural products such as sliced radish, potato, carrot, and oyster mushroom. Drying characteristics of agricultural products in solar drying system were compared with those of indoor and outdoor ones. Results: Solar drying system showed considerable effect on reducing the half drying time for all drying samples. However, outdoor drying was more effective than indoor drying on shortening the half drying time for all of drying samples. Solar drying system and outdoor drying for oyster mushroom showed the same half drying time. Conclusions: Oyster mushroom could be dried easily under outdoor drying until MR (Moisture Ratio) was reached to about 0.2. However, solar drying system showed great effect on drying for most samples compared with indoor and outdoor dryings, when MR was less than 0.5.

• 대한전자공학회논문지
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• 제19권2호
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• pp.14-22
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• 1982

국내 최초로 대구경 카세그레인 안테나의 자체 설계및 제작기술을 연구하고 시작품에 대한 성능을 측정 비교하였다. 카세그레인 안테나의 설계에 있어서는 여러 문헌을 참고하여 그 설계 수순을 정하고 특히 선진국에서 인공위성으로 부터의 TV전파 직접수신용으로 지목하고 있는 직경 4.6m인 파라보라회사 반대 곡면형 카세그레인 안테나의 제작에 있어 파라보라 곡면의 12분의 1 크기의 소곡면의 정밀제작및 이들의 정밀조립에 힘썼고 주어진 복반사경에 대하여 일차복사기의 개구 크기와 위치가 최소차폐를 만족하도록 전산 설계하는데 주력하였다. 시작된 안테나의 제성능은 이득이 43dB, 최대 정재파비 1.15, 판치각 1.1°등으로 나타났으며 같은 유형의 외국제품에 비하여 천색이 없었다.

• 한국태양에너지학회 논문집
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• 제27권4호
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• pp.113-120
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• 2007

The 5kWt dish solar collector is designed and the preliminary performance test for this is carried out. The diameter of the parabolic dish is 3.2 m, and its focal length is 2 m. It consists of 10 small reflectors which have their own curvatures, and the effective reflecting area is $5.9\;m^2$, and the rim angle of the dish is $43.85^{\circ}$. The reflectivity of reflectors is 0.95, and the thermal capacity of the system is about 5 kW thermal. The aperture diameter of the cylindrical-shape receiver which is made of stainless steel is 100 mm, and the height is 210 mm. A quartz window is installed at the receiver aperture to minimize the convective heat loss and prevent air leakage. In order to increase the heat transfer area, porous materials (nickel-alloy) are inserted into the receiver. Air flows into the upper part of the receiver which is the opposite side of the aperture. After the air flows through the inside of the receiver, that goes out of the receiver through 3 exits which are located near the aperture. The volumetric flow rates of air are varied from 600 to 1200 L/min. The results show that the system efficiency and receiver efficiency increase as the volume flow rate increases.

• 한국광학회지
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• 제22권1호
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• pp.16-22
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• 2011

중적외선 결상용 실리콘 렌즈의 변조전달함수(MTF)를 칼날 주사방식으로 측정하는 적외선 MTF 측정장치를 구성하였다. 이를 위하여 반달형 칼날 물체를 사용하여 초점거리 50 mm, F/4인 실리콘 렌즈에 대한 중적외선 파장대인 $3{\sim}5\;{\mu}m$에서의 축상 자오 방향에 대한 MTF를 측정하였다. 이 때 무한 물체를 만들기 위해서 초점거리가 2.545 m인 비축 포물 반사경을 사용하였다. 측정한 MTF는 렌즈의 설계 자료로부터 구한 MTF와 비교한 결과, 7 lp/mm 이하에서 2 % 이내의 MTF 허용오차를 만족하고 있음을 알 수 있었다.